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Observations of Markarian 421 by the CAT imaging telescope

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dc.contributor.author Fleury, P
dc.date.accessioned 2008-06-13T06:22:28Z
dc.date.available 2008-06-13T06:22:28Z
dc.date.issued 2002
dc.identifier.citation BASI, Vol. 30, No. 1, pp. 291 - 296 en
dc.identifier.uri http://hdl.handle.net/2248/2425
dc.description.abstract The CAT imaging telescope has been exploited since 1997 for the observation of Mrk-421 among other sources. After a brief review of the characteristics of the CAT telescope, the event reconstruction method will be described. We then present recent analysis results, with emphasis on the determination of the energy spectrum, its shape and its dependence upon the level of activity of the blazar. en
dc.format.extent 546877 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2002BASI...30..291F en
dc.subject Gamma Astronomy en
dc.subject Space Astronomy en
dc.subject Atmospheric Cherenkov Detectors en
dc.title Observations of Markarian 421 by the CAT imaging telescope en
dc.type Article en


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